Theoretical evidence of H-He demixing under Jupiter and Saturn conditions
Theoretical evidence of H-He demixing under Jupiter and Saturn conditions
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Author / Creator
Chang, Xiaoju , Chen, Bo , Zeng, Qiyu , Wang, Han , Chen, Kaiguo , Tong, Qunchao , Yu, Xiaoxiang , Kang, Dongdong , Zhang, Shen , Guo, Fangyu , Hou, Yong , Zhao, Zengxiu , Yao, Yansun , Ma, Yanming and Dai, Jiayu
Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
The immiscibility of hydrogen-helium mixture under the temperature and pressure conditions of planetary interiors is crucial for understanding the structures of gas giant planets (e.g., Jupiter and Saturn). While the experimental probe at such extreme conditions is challenging, theoretical simulation is heavily relied in an effort to unravel the mi...
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Full title
Theoretical evidence of H-He demixing under Jupiter and Saturn conditions
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TN_cdi_doaj_primary_oai_doaj_org_article_7190aab81cd24ce2b0f8ab22c25f39b6
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_7190aab81cd24ce2b0f8ab22c25f39b6
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ISSN
2041-1723
E-ISSN
2041-1723
DOI
10.1038/s41467-024-52868-4
